# A Quantum Window Onto Early Inflation

**Authors:** Robert J. Hardwick, Vincent Vennin, David Wands

arXiv: 1705.05746 · 2017-11-22

## TL;DR

Quantum corrections to early Universe inflation dynamics enable probing much earlier epochs than classical models, expanding our observational window into the high-energy regime of gravity during inflation.

## Contribution

This paper introduces the idea that quantum effects extend the observable window of inflationary dynamics into earlier epochs, beyond classical limitations.

## Key findings

- Quantum corrections influence cosmological fluctuation statistics.
- Spectator field displacements are sensitive to earlier inflationary phases.
- The observable inflationary window can be extended by many orders of magnitude.

## Abstract

Inflation in the early Universe is one of the most promising probes of gravity in the high-energy regime. However, observable scales give access to a limited window in the inflationary dynamics. In this essay, we argue that quantum corrections to the classical dynamics of cosmological fields allow us to probe much earlier epochs of the inflationary phase and extend this window by many orders of magnitude. We point out that both the statistics of cosmological fluctuations at observable scales, and the field displacements acquired by spectator fields that play an important role in many post-inflationary processes, are sensitive to a much longer phase of the inflationary epoch.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1705.05746/full.md

## References

26 references — full list in the complete paper: https://tomesphere.com/paper/1705.05746/full.md

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Source: https://tomesphere.com/paper/1705.05746